空间载荷机柜热控设计的仿真研究

空间站主动热控系统的作用是提供和保持航天员、仪器设备和结构部件所要求的温度、湿度和风速等热环境。本文以空间载荷机柜为热控系统的基本单元，建立了以单相流体循环回路为基础、采用液冷结合风冷的冷却方式的载荷机柜数学模型；介绍了模糊增量控制算法的工作原理；提出了采用模糊增量控制算法，以液冷支路进出口温差和风冷支路冷却量占总冷却量的比值为控制目标的反馈控制策略。同时文章采用数值模拟方法研究了控制系统的动态响应效果。仿真结果显示，模糊增量控制算法具有响应迅速、超调量小、无静态误差的特点，控制策略满足有效性、稳定性和高精确度的要求。     

基于梯度提升决策树的量子科学实验卫星光学实验预测

量子科学实验卫星在轨运行期间完成4种光学实验，地面监测人员通过遥测参数阈值判断卫星是否进行光学实验、实验类型及实验结果.这种方法需要预先设定大量阈值，并且这些阈值需要根据在轨卫星重新设定，可扩展性较差.针对以上问题，提出一种基于机器学习的光学实验判别方法，将量子科学实验卫星的光学实验监测任务抽象为机器学习中的多元分类问题，构建分类模型，利用量子科学实验卫星的真实历史遥测数据对模型进行训练，并通过真实实验计划对训练得到的模型进行验证.实验结果表明，本文提出的方法在没有专家先验知识的前提下，判别准确率达到99%，可用于量子科学实验卫星光学实验的实时监测任务.提出的基于机器学习的判别方法具有较强的可扩展性，可应用于卫星在轨运行的其他监测任务.      

First estimations of the aerosol optical thickness using Langley Method at Southern Brazil (29.4°S, 53.8°W)

The first estimations of the aerosol optical thickness (AOT) using Langley Method at Southern Space Observatory (SSO) at Southern Brazil (29.4°S, 53.8°W) are presented. In addition to ozone and sulphur dioxide columns, AOT can be obtained using Brewer Spectrophotometer at specific wavelengths: 306.3, 310.1, 313.5, 316.8 and 320.1 nm. The AOT was obtained for the period from November/2002 to May/2003. Very low AOT averages were obtained, whose values were about 0.21 ± 0.03 at 306.3 nm, 0.21 ± 0.02 at 310.1 nm, 0.19 ± 0.02 at 313.5 nm, 0.20 ± 0.02 at 316.8 nm and 0.20 ± 0.02 at 320.0 nm for all period analysed. Different behaviour of AOT were obtained at two daily specific periods of aerosol accumulation, one in the afternoons from November/2002 to February/2003, caused mainly by a mild biomass burning season’s in the region and other in the mornings from March to May/2003, due the high relative humidity presented in the region studied.     

Scientific Planning and Commanding of the Rosetta Payload

ESA’s Rosetta mission was launched in March 2004 and is on its way to comet 67P/Churyumov-Gerasimenko, where it is scheduled to arrive in summer 2014. It comprises a payload of 12 scientific instruments and a Lander. All instruments are provided by Principal Investigators, which are responsible for their operations. As for most ESA science missions, the ground segment of the mission consists of a Mission Operations Centre (MOC) and a Science Operations Centre (SOC). While the MOC is responsible for all spacecraft-related aspects and the final uplink of all command timelines to the spacecraft, the scientific operations of the instruments and the collection of the data and ingestion into the Planetary Science Archive are coordinated by the SOC. This paper focuses on the tasks of the SOC and in particular on the methodology and constraints to convert the scientific goals of the Rosetta mission to operational timelines.     

光学中心偏测量仪软件研制

文章介绍了北京空间机电研究所自行研制的光学中心偏测量仪的软件设计思路、工作原理 ,并对一些关键技术进行了讨论。     

航天光学相机地面测控设备通用化研究

文章提出了航天光学相机控制系统测试设备通用化研究的思路，制定了通用化方案，对各功能模块进行了通用化设计。     

光纤嵌入法监测复合材料固化的研究

通过嵌入光纤对芳纶／五氧复合材料板及环氧树脂浇注体的固化进行初步研究，结果表明，光纤嵌入法能准确监测出浇注体及芳纶／环氧复合材料的瞬时固化情况。     

卫星微波遥感定标技术

在简要论述微波遥感定标技术工作特点的基础上，着重分析星载有源微波遥感定标技术基本原理和关键技术，比较了各种定标方法特点，提出了若干建议。     

CBERS-1卫星CCD相机光学系统设计

CBERS -1卫星CCD相机的光学系统采用了折射式光学系统。文章介绍了该系统的设计特点     

航天光学采样成像系统MTF的优化设计与MTFC

简要介绍了成像链、成像系统和遥感系统的概念；对像质和像质差异的表征和度量、成像系统性能的表征等予以说明；重点探讨航天光学采样成像系统MTF的优化设计与MTFC问题，并给出讨论结果。